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The Dovyren intrusive complex (northern Baikal region, Russia): Isotope-geochemical markers of contamination of parental magmas and extreme enrichment of the source

Citation

Ariskin, AA and Danyushevsky, LV and Konnikov, EG and Maas, R and Kostitsyn, YA and McNeill, A and Meffre, S and Nikolaev, GS and Kislov, EV, The Dovyren intrusive complex (northern Baikal region, Russia): Isotope-geochemical markers of contamination of parental magmas and extreme enrichment of the source, Russian Geology and Geophysics, 56, (3) pp. 411-434. ISSN 1068-7971 (2015) [Refereed Article]

Copyright Statement

Copyright 2015 V.S. Sobolev IGM, Siberian Branch of the RAS.

DOI: doi:10.1016/j.rgg.2015.02.004

Abstract

The Dovyren intrusive complex includes the ore-bearing (Cu–Ni–PGE) Yoko–Dovyren layered pluton (728 Ma, up to 3.4 km in thickness), underlying ultramafic sills, and comagmatic leuconorite and gabbro-diabase dikes. Studies of Sr–Nd–Pb isotope systems were carried out for 24 intrusive rocks and five associated low- and high-Ti basalts. The high-Ti basalts show 0.7028 ≤ (87Sr/86Sr)T ≤ 0.7048 and 4.6 ≤ εNd(T) ≤ 5.8, similar to the values in MORB. The intrusive basic and ultrabasic rocks are geochemically similar to the low-Ti formation, making a compact cluster of compositions with extremely high ratios of radiogenic Sr and Pb isotopes and low εNd values. The maximum enrichment in radiogenic Sr is shown by the rocks near the pluton bottom ((87Sr/86Sr)T = 0.71387 ± 0.00010 (2σ); εNd(T) = –16.09 ± 0.06), which are the products of crystallization of the most primitive high-Mg magmas. The above-located dunites, troctolites, and gabbro show lower enrichment, probably because of the contamination of the host rocks during the filling of the magma chamber and/or because of the slight heterogeneity of the source. Calculations of the proportions of mixing of the parental melt with carbonate terrigenous material have shown that the variations in the Sr and Nd isotope ratios are due to the incredibly high contamination of the sediments, up to 40–50%. This contradicts the succession of the main rock types in the Yoko–Dovyren pluton in accordance with the crystallization of picrite-basaltic magma. The contribution of 5–10% high-Ti component seems more likely and suggests interaction between two isotopically contrasting magmas in this province in the Late Riphean. In general, the minor variations in εNd(T) of the intrusive rocks and metavolcanics (–14.3 ± 1.1) testify to the isotopically anomalous source of the low-Ti magmas. The time variation trend of εNd and geochemical features of the Dovyren rocks indicate that the products of melting of 2.7–2.8 Ga suprasubduction mantle might have been the massif protolith. Thus, the Dovyren parental magmas formed from a much older (sub)lithospheric source in the Late Riphean. The source was initially enriched in a mafic component with a low Sm/Nd ratio and was isolated from the convecting mantle and mantle melting processes for ~ 2 Gyr. The existence of such a long-living and at least twice reactivated lithospheric substratum is confirmed by the fact that the Nd isotope evolution trend of the initially nonanomalous mantle protolith includes not only the Dovyren rocks but also the Paleoproterozoic gabbro of the Chinei pluton and the Archean enderbites of the Baikal region.

Item Details

Item Type:Refereed Article
Keywords:igneous petrology, geochemistry, Cu-Ni-PGE mineralization, Sr-Nd-Pb system, extreme enrichment, anomalous mantle, ancient lithospheric source, renewed activity, Dovyren intrusive complex, Siberian craton
Research Division:Earth Sciences
Research Group:Geochemistry
Research Field:Isotope Geochemistry
Objective Division:Expanding Knowledge
Objective Group:Expanding Knowledge
Objective Field:Expanding Knowledge in the Earth Sciences
Author:Danyushevsky, LV (Professor Leonid Danyushevsky)
Author:McNeill, A (Dr Andrew McNeill)
Author:Meffre, S (Dr Sebastien Meffre)
ID Code:105856
Year Published:2015
Funding Support:Australian Research Council (CE0561595)
Web of Science® Times Cited:5
Deposited By:Centre for Ore Deposit Research - CODES CoE
Deposited On:2016-01-18
Last Modified:2017-10-24
Downloads:0

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